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- W2029588411 abstract "Abstract Some effects of energy flow and energy dissipation in an ionospheric model simulated with the Monte Carlo method, were calculated. In this model, which is described in detail in a previous paper, the trajectories of photons with a wavelength between 10 and 1027 A, and the following photoelectrons, were traced through the atmosphere between 1000 and 120km. Height dependent values of the electron and the neutral gas heating efficiency were presented. For the latter quantity a photon wavelength dependence is also given. The calculations were performed for a case of low and a case of high solar activity." @default.
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- W2029588411 title "Monte Carlo simulation of a model ionosphere—II. Energy flow and energy dissipation" @default.
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- W2029588411 doi "https://doi.org/10.1016/0021-9169(73)90033-0" @default.
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